![Evolution of a dwarf galaxy in the NIHAO simulations. The images show the gas temperature (red is hot, blue is cold) at different redshift. One can appreciate the hot bubble of gas driven away from supernovae explosions. Credit: NIHAO collaboration.
Evolution of a dwarf galaxy in the NIHAO simulations. The images show the gas temperature (red is hot, blue is cold) at different redshift. One can appreciate the hot bubble of gas driven away from supernovae explosions. Credit: NIHAO collaboration.](/sites/default/files/styles/crop_square_2_2_to_320px/public/images/gallery/news/prensa1414_3261.jpg?itok=APt3XUZY)
An international team of astronomers, led by an ex‐student of the University of La Laguna (ULL), José R. Bermejo‐Climent, and a researcher at the Instituto de Astrofísica de Canarias (IAC), G. Battaglia, finds that some of the small galaxies that orbit around the Milky Way could modify the inner structure of their dark matter haloes already in the first phases of their life due to the energy produced by supernovae explosions.
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